Galaxy Rotation Curves as a probe of Chameleon-Screened Scalar Fields
David F. Mota
TL;DR
This paper investigates how galaxy rotation curves can be used to test theories involving chameleon-screened scalar fields, aiming to understand modifications to gravity at galactic scales.
Contribution
It proposes a novel method to use galaxy rotation data to constrain chameleon scalar field models in modified gravity theories.
Findings
Constraints on chameleon field parameters from galaxy rotation curves
Potential to distinguish screened modified gravity from dark matter models
Framework for future observational tests
Abstract
This paper has been withdrawn by the author due to a mistake.
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Taxonomy
TopicsGeophysics and Gravity Measurements · Astronomy and Astrophysical Research · Stellar, planetary, and galactic studies